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Volumn 305, Issue 5690, 2004, Pages 1582-1586

Jupiter's atmospheric composition from the Cassini thermal infrared spectroscopy expirement

(42)  Kunde, V G a   Flasar, F M b   Jennings, D E b   Bezard B c   Strobel, D F d   Conrath, B J e   Nixon, C A a   Bjoraker, G L b   Romani, P N b   Achterberg, R K f   Simon Miller, A A b   Irwin, P g   Brasunas, J C b   Pearl, J C b   Smith, M D b   Orton, G S h   Gierasch, P J e   Spilker, L J h   Carlson, R C f   Mamoutkine, A A f   more..


Author keywords

[No Author keywords available]

Indexed keywords

ACETYLENE; ATMOSPHERICS; CARBON DIOXIDE; ETHANE; MORPHOLOGY; SPACECRAFT; UPPER ATMOSPHERE;

EID: 4644307629     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.1100240     Document Type: Article
Times cited : (60)

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    • note
    • M. H. Elliott, J. S. Tingley, and F. Carroll assisted with instrument commanding and data processing. P. J. Schinder computed the pointing geometry files for the CIRS observations during the Jupiter swing-by. We acknowledge the assistance of many individuals in the planning and execution of the Jupiter science sequences. This work was supported by funding from the NASA Cassini Project for U.S. coauthors. British coauthors at Oxford and Cardiff Universities acknowledge support of the Partide Physics and Astronomy Research Council French coauthors acknowledge financial support from the Centre National d'Etudes Spatiales (CNES) and the Institut National des Sciences de l'Univers (CNRS/INSU). Comments by two reviewers substantially improved the manuscript.


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